Added actions in the 'Edit' menu and in the 'Target Editor' to update target(s) with latest Simbad information;
added an auto-update check when loading an asprox file to propose the update of all targets

Bug fixes:

Use proper geocentric positions for stations and array center in OI_ARRAY (FITS)

Version 0.9.9.5

Always use the instrument default value for the Total Integration Time on the UV Coverage Panel

Added MATISSE for ESO Period 103 (offered modes & noise parameters)

Added scale / rotation fields in the 'Target Editor' to adjust user models (FITS images):
these optional fields are taken into account in the Fits image viewer, UV Coverage panel and OIFits viewer (GUI) and by the command line tool

Added 'Mag conv.' action in the Target Editor to open the Magnitude to Flux converter (Jy to mag), useful for MATISSE fluxes

Added GetStar action in the Target Editor to open the GetStar web page for the current target

Added support of target groups (OB, user) & their target associations (OB) in the Target Editor

Restored old approach to estimate V2 / T3 error and noisy data when SNR < 3: numerical approach (sampling) does not work in such degenerated cases,
so the theoretical error are used instead (added noise to V2 / T3 data is uncorrelated)

Improved the noise modelling to compute the strehl ratio per spectral channel
and taking into account the target elevation (r0)

Improved tooltip in the UV Coverage panel to add air mass, azimuth and elevation for each sampled UV point

Added tooltip on the date field: 'the given date is used to determine the coming night at the observatory in the [DD; DD+1] range.
for example, '2014/4/4' corresponds to the night between April 4th and 5th'

Added a marker at midnight (Local time) in
the Observability panel indicating the appropriate date range [DD; DD+1] corresponding to the current night

Added Local time support in
the Observability, UV Coverage and Preferences panels. It provides the local time at the observatory
(timezone including Daylight Saving Time)

Added proper handling of the VLTI VCM pressure constraint on the Observability plot using transparent overlays representing 2.5, 2.75 and 3.0 bar.
It only indicates that the pupil may be not well corrected (flux / FoV loss); see Observability "Details" for more information

Added a new warning indicating that the VLTI VCM pressure is higher than 2.5 bar

Improved the interferometer configuration to associate a delay line and a channel to each station and describe VLTI setup more accurately (switchyard)

Modified OIFits ARRNAME values to have the interferometer name only (VLTI, not VLTI Period ...)

Modified OIFits INSNAME values to have a meaningfull instrument mode description: Instrument_lambdaFirst-lambdaLast-Nch;
lambdaFirst, lambdaLast, N are respectively the wavelength of the first and last spectral channels, the number of spectral channels
(for example: AMBER_1.48347-2.52552-37ch)

Modified evaluation of moon avoidance rules to use target fluxes (V)

Added configuration integrity checks (checksum): if file(s) modified then show a warning message at startup
and also in the JMMC legal notice on plots (Use at your own risks)

Added action 'Configuration Release Notes' in the Help menu

Enhanced the target axis on the observability plot to adjust its font size according to the number of visible items (auto fit)

Added a 'Find' feature (Previous / Next) to select a target in the target list by pattern matching on its name

Added minimal Fits CUNIT keyword support to handle angle and wavelength conversions (deg, arcsec to rad) and (nm or micron to meter)

Enabled parallelization of the observability computation in multi configuration mode

Enhanced parallelization of the Best PoPs algorithm

Fixed the color scale on UV coverage plot to use degrees instead of radians when representing the model phase

Changed Observability plot to show HA constraints, moon avoidance and wind restriction using translucent area and dotted outline

Added the symbol [i] after target names on the observability plot to indicate that
this target has user notes and show its content in the observability tooltip

Added HA constraints (per target) in the observability computation displayed using translucent area and dotted outline

Added a combo box in the main settings to see estimated best Pops combinations and their effect on observability

Enhanced the Best PoPs algorithm to take new rules into account (transit distance and HA constraints);
it is based on a normal law estimator that allows more control (gaussian variance and average estimation versus min estimation)

Made the color scale on UV coverage plot interactive to show only effective data range (even when zooming in/out)

Added preferences for night only and best PoPs algorithms (Simple, Transit or HALimits)

Added preliminary support for the Sydney University Stellar Interferometer (SUSI) with PAVO instrument (2T)

Enhanced JSkyCalc interoperability to provide complete target list as an object list
that are all plotted on the sky display and airmass plots

Added sky button on the main panel to open JSkyCalc which provides sky display (moon, planets),
airmass plots and many other features for the current target and date

Added preliminary MATISSE instrument to VLTI Future Period

Added pointing restrictions due to the Moon when night restrictions are enabled to find nights without any problem.
A warning message gives the minimum angular separation and its corresponding time; use Details on the Observability plot to see its impact

Added the timeline (red line) on the observability plot to indicate the system current time (useful during real observations)

Added 'Night only' option on the observability plot to automatically zoom and focus on the night

Added OI_VIS table in the OIFits output even if the instrument is not AMBER;
it contains correlated fluxes VISDATA/VISERR anyway but VISAMP/VISPHI are set to NaN for other instruments because Aspro2 does not know
how these quantities are computed by each instrument data reduction software

Support standard SAMP 'load.votable' message to get targets in VOTable format (topcat for example)

Use an hour angle axis when the observability displays the baseline limits

Normalize model flux weights to compute visibilities

Added CHARA instruments: CLASSIC (2T) and CLIMB (3T)

Better exception handling and user messages

Unexpected exceptions are now propagated to the feedback report

Added 'Aspro 2 / JMMC' label on plots

Fixed FT_SENSOR value (FINITO or NONE) in AMBER Observing blocks

Remove Astrogrid Pal library

Fixed memory leak related to Preference listeners

Offical release of Aspro 2

Bug fixes:

Limit the memory footprint when the sampling periodicity is very small (less than 1 minute).
First 500 HA samples are computed and the following warning is displayed: 'Too many HA points (...), check your sampling periodicity. Only 500 samples computed'

Fixed bug when the UV Max value is set to 0.
This slider has now a minimum value set to the smallest baseline length of the selected interferometer